2017 VV is a very small asteroid whose orbit crosses the orbit of Earth. NASA JPL has classified 2017 VV as a "Potentially Hazardous Asteroid" due to its predicted close pass(es) with Earth.
2017 VV orbits the sun every 887 days (2.43 years), coming as close as 0.83 AU and reaching as far as 2.78 AU from the sun. Based on its brightness and the way it reflects light, 2017 VV is probably between 0.216 to 0.483 kilometers in diameter, making it a small to average asteroid, very roughly comparable in size to a football field.
2017 VV's orbit is 0.02 AU from Earth's orbit at its closest point. This means that there is a wide berth between this asteroid and Earth at all times.
2017 VV has 6 close approaches predicted in the coming decades:
Date | Distance from Earth (km) | Velocity (km/s) |
---|---|---|
May 15, 2022 | 9,254,190 | 18.272 |
May 20, 2039 | 3,395,280 | 16.557 |
May 15, 2095 | 11,198,959 | 18.531 |
May 26, 2112 | 13,436,654 | 14.948 |
May 16, 2168 | 9,040,246 | 18.169 |
May 26, 2185 | 13,882,108 | 14.889 |
2017 VV's orbit is determined by observations dating back to March 6, 2017. It was last officially observed on Nov. 2, 2022. The IAU Minor Planet Center records 162 observations used to determine its orbit.
The position of 2017 VV is indicated by a ◯ pink circle. Note that the object may not be in your current field of view. Use the controls below to adjust position, location, and time.
The below comparison is an artistic rendering that uses available data on the diameter of 2017 VV to create an approximate landscape rendering with New York City in the background. This approximation is built for full-resolution desktop browsers. Shape, color, and texture of asteroid are imagined.